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Double beta decay is indispensable to solve the question of the neutrino mass matrix together with $\nu$ oscillation experiments. Recent analysis of the most sensitive experiment since nine years - the HEIDELBERG-MOSCOW experiment in…

High Energy Physics - Phenomenology · Physics 2014-11-17 H. V. Klapdor-Kleingrothaus

The observation of neutrinoless double beta decay will have important consequences. First it will signal that lepton number is not conserved and the neutrinos are Majorana particles. Second, it represents our best hope for determining the…

High Energy Physics - Phenomenology · Physics 2016-12-12 J. D. Vergados , H. Ejiri , F Šimkovic

Future galactic supernovae will provide an extremely long baseline for studying the properties and interactions of neutrinos. In this paper, we discuss the possibility of using such an event to constrain (or discover) the effects of exotic…

High Energy Astrophysical Phenomena · Physics 2010-10-01 Chris Kelso , Dan Hooper

In this review we discuss the current status of research in nuclear physics which is being carried out in different centers in the World. For this purpose we supply a short account of the development in the area which evolved over the last…

Nuclear Theory · Physics 2017-03-22 C. A. Bertulani , M. S. Hussein

The first evidence for neutrinoless double beta decay has been observed in the HEIDELBERG-MOSCOW experiment, which is the most sensitive double beta decay experiment since ten years. This is the first evidence for lepton number violation…

High Energy Physics - Phenomenology · Physics 2017-08-23 H. V. Klapdor-Kleingrothaus

The motivation for the search for $0\nu\beta\beta$ decay is briefly reviewed. It is stressed that the exchange of light Majorana neutrinos is not the only possible mechanism of the decay. The link between lepton number and lepton flavor…

High Energy Physics - Phenomenology · Physics 2008-07-11 Petr Vogel

The primary motivation for building neutrino telescopes is to open the road for neutrino astronomy, and to offer another observational window for the study of cosmic ray origins. Other physics topics, such as the search for WIMPs, can also…

Astrophysics · Physics 2019-08-13 Cecile Portello-Roucelle

Three facets of symmetries in neutrino physics are briefly reviewed: i) The SO(5) symmetry of the neutrino mass and and its connection to the see-saw mechanism; ii) Flavor SU(N) symmetries of dense, self-interacting neutrino gases in…

Nuclear Theory · Physics 2014-11-20 A. B. Balantekin

In the first Lecture, the Big Bang and the Standard Model of particle physics are introduced, as well as the structure of the latter and open issues beyond it. Neutrino physics is discussed in the second Lecture, with emphasis on models for…

Astrophysics · Physics 2007-05-23 John Ellis

Core-collapse supernovae are powerful neutrino sources. The observation of a future (extra-)galactic supernova explosion or of the relic supernova neutrinos might provide important information on the supernova dynamics, on the supernova…

Astrophysics · Physics 2009-11-13 J. Gava , C. Volpe

I review the physics of the Diffuse Supernova Neutrino flux (or Background, DSNB), in the context of future searches at the next generation of neutrino observatories. The theory of the DSNB is discussed in its fundamental elements, namely…

Cosmology and Nongalactic Astrophysics · Physics 2016-05-24 Cecilia Lunardini

The neutrino physics program at the LHC, which will soon be initiated by the FASER experiment, will provide unique opportunities for precision studies of neutrino interaction vertices at high energies. This will also open up the possibility…

High Energy Physics - Phenomenology · Physics 2021-05-25 Krzysztof Jodłowski , Sebastian Trojanowski

Astrophysics is gaining increased attention from the particle and nuclear physics communities, as budget cuts, delays, and cancellations limit opportunities for breakthrough research at accelerator laboratories. Observations of cosmic rays…

Astrophysics · Physics 2009-10-22 R. Jeffrey Wilkes

We study the neutrino oscillation physics performance of the Long-Baseline Neutrino Experiment (LBNE) in various configurations. In particular, we compare the case of a surface detector at the far site augmented by a near detector, to that…

High Energy Physics - Phenomenology · Physics 2014-01-22 Vernon Barger , Atri Bhattacharya , Animesh Chatterjee , Raj Gandhi , Danny Marfatia , Mehedi Masud

Astroparticle physics is a field rich of perspectives in investigating the ultra-high energy region which will never be accessible to man made machines. Many efforts are underway in order to detect the first cosmic neutrinos, messengers of…

Astrophysics · Physics 2022-02-23 Teresa Montaruli

Neutron stars are some of the densest manifestations of massive objects in the universe. They are ideal astrophysical laboratories for testing theories of dense matter physics and provide connections among nuclear physics, particle physics…

Astrophysics · Physics 2011-05-05 J. M. Lattimer , M. Prakash

We discuss in detail the physics reach of an experimental set-up where electron neutrinos (anti-neutrinos) produced in a beta-beam facility at Fermi National Accelerator Laboratory (FNAL) are sent, over a distance of L~1300km, to the Deep…

High Energy Physics - Phenomenology · Physics 2015-03-13 Sanjib Kumar Agarwalla , Patrick Huber

A study of the current status of WIMP dark matter searches has been made in the context of scientific and technical planning for a Deep Underground Science and Engineering Laboratory (DUSEL) in the U.S. The table of contents follows: 1.…

The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for…

Instrumentation and Detectors · Physics 2023-02-10 J. Aalbers , K. Abe , V. Aerne , F. Agostini , S. Ahmed Maouloud , D. S. Akerib , D. Yu. Akimov , J. Akshat , A. K. Al Musalhi , F. Alder , S. K. Alsum , L. Althueser , C. S. Amarasinghe , F. D. Amaro , A. Ames , T. J. Anderson , B. Andrieu , N. Angelides , E. Angelino , J. Angevaare , V. C. Antochi , D. Antón Martin , B. Antunovic , E. Aprile , H. M. Araújo , J. E. Armstrong , F. Arneodo , M. Arthurs , P. Asadi , S. Baek , X. Bai , D. Bajpai , A. Baker , J. Balajthy , S. Balashov , M. Balzer , A. Bandyopadhyay , J. Bang , E. Barberio , J. W. Bargemann , L. Baudis , D. Bauer , D. Baur , A. Baxter , A. L. Baxter , M. Bazyk , K. Beattie , J. Behrens , N. F. Bell , L. Bellagamba , P. Beltrame , M. Benabderrahmane , E. P. Bernard , G. F. Bertone , P. Bhattacharjee , A. Bhatti , A. Biekert , T. P. Biesiadzinski , A. R. Binau , R. Biondi , Y. Biondi , H. J. Birch , F. Bishara , A. Bismark , C. Blanco , G. M. Blockinger , E. Bodnia , C. Boehm , A. I. Bolozdynya , P. D. Bolton , S. Bottaro , C. Bourgeois , B. Boxer , P. Brás , A. Breskin , P. A. Breur , C. A. J. Brew , J. Brod , E. Brookes , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , T. K. Bui , S. Burdin , S. Buse , J. K. Busenitz , D. Buttazzo , M. Buuck , A. Buzulutskov , R. Cabrita , C. Cai , D. Cai , C. Capelli , J. M. R. Cardoso , M. C. Carmona-Benitez , M. Cascella , R. Catena , S. Chakraborty , C. Chan , S. Chang , A. Chauvin , A. Chawla , H. Chen , V. Chepel , N. I. Chott , D. Cichon , A. Cimental Chavez , B. Cimmino , M. Clark , R. T. Co , A. P. Colijn , J. Conrad , M. V. Converse , M. Costa , A. Cottle , G. Cox , O. Creaner , J. J. Cuenca Garcia , J. P. Cussonneau , J. E. Cutter , C. E. Dahl , V. D'Andrea , A. David , M. P. Decowski , J. B. Dent , F. F. Deppisch , L. de Viveiros , P. Di Gangi , A. Di Giovanni , S. Di Pede , J. Dierle , S. Diglio , J. E. Y. Dobson , M. Doerenkamp , D. Douillet , G. Drexlin , E. Druszkiewicz , D. Dunsky , K. Eitel , A. Elykov , T. Emken , R. Engel , S. R. Eriksen , M. Fairbairn , A. Fan , J. J. Fan , S. J. Farrell , S. Fayer , N. M. Fearon , A. Ferella , C. Ferrari , A. Fieguth , A. Fieguth , S. Fiorucci , H. Fischer , H. Flaecher , M. Flierman , T. Florek , R. Foot , P. J. Fox , R. Franceschini , E. D. Fraser , C. S. Frenk , S. Frohlich , T. Fruth , W. Fulgione , C. Fuselli , P. Gaemers , R. Gaior , R. J. Gaitskell , M. Galloway , F. Gao , I. Garcia Garcia , J. Genovesi , C. Ghag , S. Ghosh , E. Gibson , W. Gil , D. Giovagnoli , F. Girard , R. Glade-Beucke , F. Glück , S. Gokhale , A. de Gouvêa , L. Gráf , L. Grandi , J. Grigat , B. Grinstein , M. G. D. van der Grinten , R. Grössle , H. Guan , M. Guida , R. Gumbsheimer , C. B. Gwilliam , C. R. Hall , L. J. Hall , R. Hammann , K. Han , V. Hannen , S. Hansmann-Menzemer , R. Harata , S. P. Hardin , E. Hardy , C. A. Hardy , K. Harigaya , R. Harnik , S. J. Haselschwardt , M. Hernandez , S. A. Hertel , A. Higuera , C. Hils , S. Hochrein , L. Hoetzsch , M. Hoferichter , N. Hood , D. Hooper , M. Horn , J. Howlett , D. Q. Huang , Y. Huang , D. Hunt , M. Iacovacci , G. Iaquaniello , R. Ide , C. M. Ignarra , G. Iloglu , Y. Itow , E. Jacquet , O. Jahangir , J. Jakob , R. S. James , A. Jansen , W. Ji , X. Ji , F. Joerg , J. Johnson , A. Joy , A. C. Kaboth , A. C. Kamaha , K. Kanezaki , K. Kar , M. Kara , N. Kato , P. Kavrigin , S. Kazama , A. W. Keaveney , J. Kellerer , D. Khaitan , A. Khazov , G. Khundzakishvili , I. Khurana , B. Kilminster , M. Kleifges , P. Ko , M. Kobayashi , M. Kobayashi , D. Kodroff , G. Koltmann , A. Kopec , A. Kopmann , J. Kopp , L. Korley , V. N. Kornoukhov , E. V. Korolkova , H. Kraus , L. M. Krauss , S. Kravitz , L. Kreczko , V. A. Kudryavtsev , F. Kuger , J. Kumar , B. López Paredes , L. LaCascio , Q. Laine , H. Landsman , R. F. Lang , E. A. Leason , J. Lee , D. S. Leonard , K. T. Lesko , L. Levinson , C. Levy , I. Li , S. C. Li , T. Li , S. Liang , C. S. Liebenthal , J. Lin , Q. Lin , S. Lindemann , M. Lindner , A. Lindote , R. Linehan , W. H. Lippincott , X. Liu , K. Liu , J. Liu , J. Loizeau , F. Lombardi , J. Long , M. I. Lopes , E. Lopez Asamar , W. Lorenzon , C. Lu , S. Luitz , Y. Ma , P. A. N. Machado , C. Macolino , T. Maeda , J. Mahlstedt , P. A. Majewski , A. Manalaysay , A. Mancuso , L. Manenti , A. Manfredini , R. L. Mannino , N. Marangou , J. March-Russell , F. Marignetti , T. Marrodán Undagoitia , K. Martens , R. Martin , I. Martinez-Soler , J. Masbou , D. Masson , E. Masson , S. Mastroianni , M. Mastronardi , J. A. Matias-Lopes , M. E. McCarthy , N. McFadden , E. McGinness , D. N. McKinsey , J. McLaughlin , K. McMichael , P. Meinhardt , J. Menéndez , Y. Meng , M. Messina , R. Midha , D. Milisavljevic , E. H. Miller , B. Milosevic , S. Milutinovic , S. A. Mitra , K. Miuchi , E. Mizrachi , K. Mizukoshi , A. Molinario , A. Monte , C. M. B. Monteiro , M. E. Monzani , J. S. Moore , K. Morå , J. A. Morad , J. D. Morales Mendoza , S. Moriyama , E. Morrison , E. Morteau , Y. Mosbacher , B. J. Mount , J. Mueller , A. St. J. Murphy , M. Murra , D. Naim , S. Nakamura , E. Nash , N. Navaieelavasani , A. Naylor , C. Nedlik , H. N. Nelson , F. Neves , J. L. Newstead , K. Ni , J. A. Nikoleyczik , V. Niro , U. G. Oberlack , M. Obradovic , K. Odgers , C. A. J. O'Hare , P. Oikonomou , I. Olcina , K. Oliver-Mallory , A. Oranday , J. Orpwood , I. Ostrovskiy , K. Ozaki , B. Paetsch , S. Pal , J. Palacio , K. J. Palladino , J. Palmer , P. Panci , M. Pandurovic , A. Parlati , N. Parveen , S. J. Patton , V. Pěč , Q. Pellegrini , B. Penning , G. Pereira , R. Peres , Y. Perez-Gonzalez , E. Perry , T. Pershing , R. Petrossian-Byrne , J. Pienaar , A. Piepke , G. Pieramico , M. Pierre , M. Piotter , V. Pizella , G. Plante , T. Pollmann , D. Porzio , J. Qi , Y. Qie , J. Qin , N. Raj , M. Rajado Silva , K. Ramanathan , D. Ramírez García , J. Ravanis , L. Redard-Jacot , D. Redigolo , S. Reichard , J. Reichenbacher , C. A. Rhyne , A. Richards , Q. Riffard , G. R. C. Rischbieter , A. Rocchetti , S. L. Rosenfeld , R. Rosero , N. Rupp , T. Rushton , S. Saha , L. Sanchez , P. Sanchez-Lucas , D. Santone , J. M. F. dos Santos , I. Sarnoff , G. Sartorelli , A. B. M. R. Sazzad , M. Scheibelhut , R. W. Schnee , M. Schrank , J. Schreiner , P. Schulte , D. Schulte , H. Schulze Eissing , M. Schumann , T. Schwemberger , A. Schwenk , T. Schwetz , L. Scotto Lavina , P. R. Scovell , H. Sekiya , M. Selvi , E. Semenov , F. Semeria , P. Shagin , S. Shaw , S. Shi , E. Shockley , T. A. Shutt , R. Si-Ahmed , J. J. Silk , C. Silva , M. C. Silva , H. Simgen , F. Šimkovic , G. Sinev , R. Singh , W. Skulski , J. Smirnov , R. Smith , M. Solmaz , V. N. Solovov , P. Sorensen , J. Soria , T. J. Sparmann , I. Stancu , M. Steidl , A. Stevens , K. Stifter , L. E. Strigari , D. Subotic , B. Suerfu , A. M. Suliga , T. J. Sumner , P. Szabo , M. Szydagis , A. Takeda , Y. Takeuchi , P. -L. Tan , C. Taricco , W. C. Taylor , D. J. Temples , A. Terliuk , P. A. Terman , D. Thers , K. Thieme , Th. Thümmler , D. R. Tiedt , M. Timalsina , W. H. To , F. Toennies , Z. Tong , F. Toschi , D. R. Tovey , J. Tranter , M. Trask , G. C. Trinchero , M. Tripathi , D. R. Tronstad , R. Trotta , Y. D. Tsai , C. D. Tunnell , W. G. Turner , R. Ueno , P. Urquijo , U. Utku , A. Vaitkus , K. Valerius , E. Vassilev , S. Vecchi , V. Velan , S. Vetter , A. C. Vincent , L. Vittorio , G. Volta , B. von Krosigk , M. von Piechowski , D. Vorkapic , C. E. M. Wagner , A. M. Wang , B. Wang , Y. Wang , W. Wang , J. J. Wang , L. -T. Wang , M. Wang , Y. Wang , J. R. Watson , Y. Wei , C. Weinheimer , E. Weisman , M. Weiss , D. Wenz , S. M. West , T. J. Whitis , M. Williams , M. J. Wilson , D. Winkler , C. Wittweg , J. Wolf , T. Wolf , F. L. H. Wolfs , S. Woodford , D. Woodward , C. J. Wright , V. H. S. Wu , P. Wu , S. Wüstling , M. Wurm , Q. Xia , X. Xiang , Y. Xing , J. Xu , Z. Xu , D. Xu , M. Yamashita , R. Yamazaki , H. Yan , L. Yang , Y. Yang , J. Ye , M. Yeh , I. Young , H. B. Yu , T. T. Yu , L. Yuan , G. Zavattini , S. Zerbo , Y. Zhang , M. Zhong , N. Zhou , X. Zhou , T. Zhu , Y. Zhu , Y. Zhuang , J. P. Zopounidis , K. Zuber , J. Zupan

This paper presents a review of the history, motivation and current status of high energy neutrino telescopes. Many years after these detectors were first conceived, the operation of kilometer-cubed scale detectors is finally on the horizon…

Astrophysics · Physics 2010-01-15 K. D. Hoffman